ar X iv : a st ro - p h / 07 02 34 5 v 1 1 3 Fe b 20 07 A procedure for the inversion of f - mode travel times for solar flows
نویسندگان
چکیده
We perform a two-dimensional inversion of f-mode travel times to determine near-surface solar flows. The inversion is based on optimally localized averaging of travel times. We use finite-wavelength travel-time sensitivity functions and a realistic model of the data errors. We find that it is possible to obtain a spatial resolution of 2 Mm. The error in the resulting flow estimate ultimately depends on the observation time and the number of travel distances used in the inversion.
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